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Outflow signatures in Gemini GMOS-IFU observations of 5 nearby Seyfert 2 galaxies
Published online by Cambridge University Press: 29 March 2021
Abstract
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We use Gemini Multi-Object Spectrograph (GMOS) Integral Field Unit (IFU) observations of a sample of 5 bright nearby Seyfert galaxies to map their emission-line flux distributions and kinematics at a spatial resolution ranging from 110 to 280 pc. For all galaxies, the gas kinematics show two components: a rotation and an outflow component.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 274 - 276
- Copyright
- © The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union
References
Schmitt, H. R., Ulvestad, J. S., Antonucci, R. R. J., et al. 2001, ApJS, 132, 199
10.1086/318957CrossRefGoogle Scholar
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